paper

Radiation gasdynamics of planetary nebulae -- VI. The evolution of aspherical planetary nebulae

arXiv:astro-ph/9506033 · doi:10.1093/mnras/277.1.173

Abstract

This paper reports the results of the numerical study of the formation of aspherical Planetary Nebulae through the Generalised Interacting Winds Model, taking into account the effects caused by the evolving central star and fast wind. The results show for the first time that aspherical nebulae do form within the required time scale. Consideration of the development of the nebula shows that in the early stages it is the ionization of the aspherical AGB wind that contributes considerably to the shaping of the nebula. Furthermore the passing through of the ionization front may modifies the density distribution in the slow wind, leading to the formation of a surrounding envelope, and sometimes a different morphology for the nebula than was to be expected from the initial conditions. I consider how the different phases of ionization fronts and wind swept bubbles can be observationally distinguished.

21 pages, uuencoded compressed Postscript, without the figures; accepted by MNRAS; also available (_with_ included figures) in ftp://axp1.ast.man.ac.uk/outgoing/gm/mn_pnVI.v2f.ps.Z and on http://saturn.ma.umist.ac.uk/Preprints2.html/

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